activity
20032009
most citedA Spitzer view of protoplanetary disks in the gamma Velorum cluster

251 citations · 706 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.SR200946 cited

The Differential Rotation of FU Ori

Zhaohuan Zhu, Catherine Espaillat, Kenneth Hinkle +3

The emission of FU Orionis objects in outburst has been identified as arising in rapidly accreting protoplanetary disks, based on a number of observational properties. A fundamenta…

astro-ph200855 cited

Long-wavelength excesses of FU Orionis objects: flared outer disks or infalling envelopes?

Zhaohuan Zhu, Lee Hartmann, Nuria Calvet +3

The mid- to far-infrared emission of the outbursting FU Orionis objects has been attributed either to a flared outer disk or to an infalling envelope. We revisit this issue using d…

astro-ph2008251 cited

A Spitzer view of protoplanetary disks in the gamma Velorum cluster

Jesus Hernandez, Lee Hartmann, Nuria Calvet +4

We present new Spitzer Space Telescope observations of stars in the young ~5 Myr gamma Velorum stellar cluster. Combining optical and 2MASS photometry, we have selected 579 stars a…

astro-ph2007195 cited

Spitzer observations of the Orion OB1 association: disk census in the low mass stars

Jesus Hernandez, Nuria Calvet, C. Briceno +6

We present new Spitzer Space Telescope observations of two fields in the Orion OB1 association. We report here IRAC/MIPS observations for 115 confirmed members and 41 photometric c…

astro-ph2007159 cited

The Hot Inner Disk of FU Ori

Zhaohuan Zhu, Lee Hartmann, Nuria Calvet +3

We have constructed a detailed radiative transfer disk model which reproduces the main features of the spectrum of the outbursting young stellar object FU Orionis from ~ 4000 angst…

astro-ph2004

Disk evolution in the Ori OB1 association

Nuria Calvet, Cesar Briceno, Jesus Hernandez +5

We analyze multi-band photometry of a subsample of low mass stars in the associations Ori OB1a and 1b discovered during the CIDA Orion Variability Survey, which have ages of 7 - 10…